High precision radial velocities of southern solar-type stars by cross-correlation

Details High precision radial velocities of southern solar-type stars by cross-correlation High precision radial velocities of southern solar-type stars by cross-correlation

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.186..169m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 186, no. 2, Dec. 1991, p. 169-177.

Physics

Optics

12

Cross Correlation, Dwarf Stars, Late Stars, Radial Velocity, Data Reduction, Echelle Gratings, Fiber Optics, Precision, Southern Sky, Stellar Spectrophotometry

Scientific paper

The present paper describes a program at the Mt. John University Observatory whose purpose is to monitor the radial velocities of 29 bright southern solar-type dwarfs at about monthly intervals in order to search for low-amplitude periodic variations. The use of a fiber-feed between the telescope and echelle spectrograph enables a stability allowing a precision of better than 50 m/s. Observations of 29 southern solar-type stars are reported.

Affiliated with

Also associated with

No associations

Rating

High precision radial velocities of southern solar-type stars by cross-correlation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High precision radial velocities of southern solar-type stars by cross-correlation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High precision radial velocities of southern solar-type stars by cross-correlation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1536561